A reciprocity for symmetric algebras

The aim of this note is to show, that the reciprocity property of group algebras in [5, (11.5)] can be deduced from formal properties of symmetric algebras, as exposed in [1], for instance

The Pulsed Neutron Beam EDM Experiment

We report on the Beam EDM experiment, which aims to employ a pulsed cold neutron beam to search for an electric dipole moment instead of the established use of storable ultracold neutrons. We present a brief overview of the basic measurement concept and the current status of our proof-of-principle Ramsey apparatus

Genetic improvement of meat quality and fertility using the national nucleus

Knowledge is power and the National Swine Registry (NSR) is the only source of complete, publicly available, genetic records on nucleus populations. NSR has offered STAGES \u27, a BLUP genetic improvement program with bio-economic indexes for over 17 years. NSR members submit information on 3 sow productivity traits and 3 postweaning performance traits and in return receive across-herd Expected Progeny Deviations (EPDs) for these traits along with indexes for Sow Productivity, Maternal Line (sow productivity and postweaning performance) and Terminal (postweaning traits only) to be used in genetic selection. Not only is this genetic information available to members but genetic values and trends for these traits are also available to any commercial producer or genetic advisor. This program has led NSR members to make substantial genetic improvement for these traits within all four breeds. In addition, this transparent system allows commercial producers to design programs and select animals that allow them the greatest potential for their situation. As the pork industry continues ro change, multiple pork chains are forming to meets distinct specifications desired by subsets of consumers. To continue to meet the demand of these dissimilar pork chains, differentiated genetic lines are necessary to provide products that match their specifications. In addition, as profit per pig continues to decline pork producers must be able to increase product sold per unit of investment. To facilitate this key profitability indicator, the fertility of breeding females must improve. To address these two key drivers in today\u27s pork industry, the NSR has updated their genetic improvement program in these two areas

The stellar mass - size relation for cluster galaxies at z=1 with high angular resolution from the Gemini/GeMS multi-conjugate adaptive optics system

We present the stellar mass - size relation for 49 galaxies within the $z$ = 1.067 cluster SPT-CL J0546$-$5345, with FWHM $\sim$80-120 mas $K_{\mathrm s}$-band data from the Gemini multi-conjugate adaptive optics system (GeMS/GSAOI). This is the first such measurement in a cluster environment, performed at sub-kpc resolution at rest-frame wavelengths dominated by the light of the underlying old stellar populations. The observed stellar mass - size relation is offset from the local relation by 0.21 dex, corresponding to a size evolution proportional to $(1+z)^{-1.25}$, consistent with the literature. The slope of the stellar mass - size relation $\beta$ = 0.74 $\pm$ 0.06, consistent with the local relation. The absence of slope evolution indicates that the amount of size growth is constant with stellar mass. This suggests that galaxies in massive clusters such as SPT-CL J0546$-$5345 grow via processes that increase the size without significant morphological interference, such as minor mergers and/or adiabatic expansion. The slope of the cluster stellar mass - size relation is significantly shallower if measured in $HST$/ACS imaging at wavelengths blueward of the Balmer break, similar to rest-frame UV relations at $z$ = 1 in the literature. The stellar mass - size relation must be measured at redder wavelengths, which are more sensitive to the old stellar population that dominates the stellar mass of the galaxies. The slope is unchanged when GeMS $K_s$-band imaging is degraded to the resolution of $K$-band HST/NICMOS resolution but dramatically affected when degraded to $K_s$-band Magellan/FourStar resolution. Such measurements must be made with AO in order to accurately characterise the sizes of compact, $z$ = 1 galaxies.Comment: 24 pages, 13 figures, 3 tables. Accepted for publication in MNRAS. Typos corrected, DOI adde

Cull Sow Feeding Management

The decision to cull a sow from the breeding herd typically occurs after weaning due to poor lactation performance, lameness or if she fails to breed or conceive. Once the decision to cull a sow from the breeding herd has been made, a producer must decide to either immediately market the sow or to increase marketable body weight by feeding her for a period of time. The decision to feed cull sows to add additional body weight is not a simple decision. Many factors such as current cull sow market prices, available housing space, feed cost, and health of the animal contribute to this decision [1]. Revenue from marketing cull sows contributes to the profitability of pork operations, therefore much care should be placed on deciding when to market cull sows